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Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars, separation of the landing module. Artist impression of separation of the ExoMars lander/rover module

Mission ExoMars - Artist view - ExoMars Mission - Artist view - Artist view of the European probe ExoMars, separation of the landing module. Artist impression of separation of the ExoMars lander/rover module

D. Ducros

PIX4606983

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

Mars surface seen by the rover Curiosity 04/2015 - Martian surface seen from the rover Curiosity 04/2015 - Panorama of the surface of Mars on Mount Sharp. Mosaic of images obtained by the rover Curiosity and his camera Mastcam on 10 and 11 April 2015. A southward - looking panorama combining images from both cameras of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars Rover shows diverse geological textures on Mount Sharp. Three years after landing on Mars, the mission is investigating this layered mountain for evidence about changes in Martian environmental conditions, from an ancient time when conditions were favorable for microbial life to the much - drier present. Gravel and sand ripples fill the foreground, typical of terrains that Curiosity traversed to reach Mount Sharp from its landing site. Outcrops in the midfield are of two types: dust - covered, smooth bedrock that forms the base of the mountain, and sandstone ridges that shed boulders as they erode. Rounded but

PIX4616735

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

Mars Science Laboratory - Mars Science Laboratory (MSL), named Curiosity, is a NASA rover to explore the surface of Mars starting in 2012. This artist concept features Nasa's Mars Science Laboratory Curiosity rover, a mobile robot for investigating Mars' past or present ability to sustain microbial life. Curiosity is being tested in preparation for launch in the fall of 2011. In this picture, the rover examines a rock on Mars with a set of tools at the end of the rover's arm, which extends about 2 meters (7 feet). Two instruments on the arm can study rocks up close. Also, a drill can collect sample material from inside of rocks and a scoop can pick up samples of soil. The arm can sieve the samples and deliver fine powder to instruments inside the rover for thorough analysis. The mast, or rover's “” head,”” rises to about 2.1 meters (6.9 feet) above ground level, about as tall as a basketball player. This mast supports two remote - sensing instruments: the Mast Camera, or “” eyes,”” for

PIX4606810

Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory

Mars Express probe - Artist's View - Mars Express artist's view - The European probe Mars Express leaves the Earth propelled by the upper floor Fregat. This probe was launched on 2 June 2003 and began its observations in early 2004. Mars Express left Earth for Mars on 2 June 2003 when the positions of the two planets made for the shortest possible route, a condition that occurs once every twenty - six months. The european spaceprobe began its March observations in 2004. Mars Express was mounted on the Fregat upper stage. Most of the energy needed to propel Mars Express from Earth to Mars is provided by the four - stage Soyuz/Fregat launcher. The Fregat upper stage separated from the spacecraft after placed it on a Mars - bound trajectory

D. Ducros

PIX4606628

Mars surface seen by the rover Curiosity 01/2014 - Martian surface seen from the rover Curiosity 01/2014 - Panorama of the surface of Mars in the crater Gale. A small sand dune one metre high is visible in the center of the image. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on January 28, 2014. This scene combines images taken by the left - eye camera of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover during the midafternoon, local Mars solar time, of the mission's 526th Martian day, or sol (Jan. 28, 2014). The sand dune in the upper center of the image spans a gap, called “” Dingo Gap,””” between two short scarps. The dune is about 3 feet (1 meter) high. The nearer edge of it is about 115 feet (35 meters) away from the top's position when the component images were taken, just after a Sol 526 drive of 49 feet (15 meters). The image has been white - balanced to show what the rocks would look like if they were on Earth

Mars surface seen by the rover Curiosity 01/2014 - Martian surface seen from the rover Curiosity 01/2014 - Panorama of the surface of Mars in the crater Gale. A small sand dune one metre high is visible in the center of the image. Mosaic of images obtained by the rover Curiosity is his Mastcam camera on January 28, 2014. This scene combines images taken by the left - eye camera of the Mast Camera (Mastcam) instrument on Nasa's Curiosity Mars rover during the midafternoon, local Mars solar time, of the mission's 526th Martian day, or sol (Jan. 28, 2014). The sand dune in the upper center of the image spans a gap, called “” Dingo Gap,””” between two short scarps. The dune is about 3 feet (1 meter) high. The nearer edge of it is about 115 feet (35 meters) away from the top's position when the component images were taken, just after a Sol 526 drive of 49 feet (15 meters). The image has been white - balanced to show what the rocks would look like if they were on Earth

PIX4616684

Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays

Artist's view of a first human crew on Mars - Martian Pioneers - The first human visitors to Mars would face an environment nearly as hostile as the Earth's Moon. While Mars has an atmosphere, it contains no breathable oxygen and is so thin that the surface air pressure is about the same as the Earth's 18 miles above sea level. To venture outside, humans would need hardy suits that would supply pressure, oxygen, moisture, warmth, and insulate them from the fine martian dust that may be both abrasive and caustic. Even with these precautions, humans would still be vulnerable to radiation from solar storms and the continual rain of interstellar cosmic rays

Walter B Myers

PIX4639821

Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

Traces of flow on Mars - Mars: gullies on impact crater wall - Gullies along a wall of an impact crater (Hale crater). These ravines are thought to indicate the presence of liquid water in the Martian basement. Image obtained by the Mars Reconnaissance Orbiter probe on August 3, 2009. Gullies, on Earth, are usually formed through the action of liquid water. Whether gullies form under today's cold dry conditions on Mars is a major question that planetary scientists are trying to answer. The gullies pictured here in Hale crater are great examples of what a typical Martian gully looks like. Wide V - shaped channels running downhill (from top to bottom) where the material that carved the gully flowed. At the bottom of the channel this material empties out onto a fan - shaped mound. Several gullies are visible here and the fans from each gully overlap one other in complicated ways. Image taken on August 3, 2009 by the HIRISE camera on Nasa's Mars Reconnaissance Orbiter

PIX4616548

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

PIX4629899

Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

Martian dunes in winter - March: Winter view of Dunes - Detail on dunes in a crater located in the southern hemisphere of Mars. Clearly, areas covered with gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on November 25, 2006. HIRISE is a 50 cm telescope that observes visible and near infrared. Dunes within a crater on Mars are visible in this HiRise image. This crater is located in the southern hemisphere where it was winter at the time this image was taken on November 25, 2006. This observation documents new seasonal processes occurring on dunes at this latitude, as well as other interesting phenomena. The bright tones are interpreted as carbon dioxide or water frost. This is generally concentrated on the east - facing slopes of the dunes, which are in shadow and therefore cooler. Some dark spots on the dunes may be areas that have defrosted more than surrounding terrain. Landslides and dark - toned streaks are seen on many of the west -

PIX4616480

Mars and its satellites seen with an amateur telescope - Mars with its moons through an amateur telescope - Composite image of the planet Mars accompanied by its two moving satellites, Phobos (left) and Deimos (right). Image taken with a C14 and a webcam on August 28, 2003 in Namibia. Composite image of planet Mars with its moons. Image taken on August 28 2003 from Namibia with a C14 telescope and a webcam. Phobos is moving on the left of the image, Deimos at right

Mars and its satellites seen with an amateur telescope - Mars with its moons through an amateur telescope - Composite image of the planet Mars accompanied by its two moving satellites, Phobos (left) and Deimos (right). Image taken with a C14 and a webcam on August 28, 2003 in Namibia. Composite image of planet Mars with its moons. Image taken on August 28 2003 from Namibia with a C14 telescope and a webcam. Phobos is moving on the left of the image, Deimos at right

Sebastian Voltmer

PIX4614913

Venus, Mars and Mercury - Venus, Mars and Mercury - Planet Mars near the brilliant Venus on the right. On the left, the planet Mercury. 13 September 2008. March close to the bright planet Venus. At left, planet Mercury. September 13 2008

Venus, Mars and Mercury - Venus, Mars and Mercury - Planet Mars near the brilliant Venus on the right. On the left, the planet Mercury. 13 September 2008. March close to the bright planet Venus. At left, planet Mercury. September 13 2008

Sebastian Voltmer

PIX4587767

Mars - Artist's View - Mars - Artwork - A view from north of Mars' equato

Mars - Artist's View - Mars - Artwork - A view from north of Mars' equato

Steven Hobbs

PIX4616817

Mars in the open cluster M44 - Planet Mars in the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. May 23, 2008. Bright Mars among M44 stars; this cluster is located about 600 light year away in Cancer. May 23, 2008

Mars in the open cluster M44 - Planet Mars in the open cluster M44 - M44 is a cluster of stars located only 600 light years from Earth, in the constellation Cancer. Illuminating the image, the planet Mars. May 23, 2008. Bright Mars among M44 stars; this cluster is located about 600 light year away in Cancer. May 23, 2008

PIX4588238

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Mars and Deimos - Illustration - Mars and Deimos - Illustration - Artist's view of Deimos, the smallest of Mars's two satellites. This is how Mars and its even smaller satellite Deimos might appear from a distance of about 100 miles from the surface of Deimos. Deimos is over Acidalia Planitia, an albedo feature that has been observed by Earth - bound astronomers since the 19th century. To the southwest are the fog - filled canyons of Valles Marineris, the westernmost of which are still in darkness. Beyond Mars, immediately to the left of its night side, is Phobos at a distance of 20,000 miles. The two bright objects in the lower left are the stars Beta Gruis and Al Nair in the southern constellation Grus. Like it's larger companion Phobos, Deimos does not possess enough mass to pull itself into a sphere; its shape instead is oblong with a length of about 10 miles and only 6 miles wide at its smallest dimension. Like Phobos, Deimos may be an asteroid long ago captured by Mars' gravity.

Walter B Myers

PIX4616824

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

The probe Mars 96 - Artist view - Mars 96 spacecraft - Artist view - Sequence of the mission of the sovietic probe Mars 96. In addition to its observations in Martian orbit, this probe was to launch two stations and two penetrators on Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Artwork showing the mission sequence of soviet March 96 spacecraft. Two surface stations and two penetrators should be deployed on the martian surface. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606454

Mars surface seen by the probe Mariner 6 - Mariner 6 closeup view of Martian craters - Martian crateres in Sinus Meridiani seen by the probe Mariner 6 in July 1969. Recolorized image. Mars craters in Sinus Meridiani seen by Mariner 6 in july 1969. Recolorized picture

Mars surface seen by the probe Mariner 6 - Mariner 6 closeup view of Martian craters - Martian crateres in Sinus Meridiani seen by the probe Mariner 6 in July 1969. Recolorized image. Mars craters in Sinus Meridiani seen by Mariner 6 in july 1969. Recolorized picture

Steven Hobbs

PIX4615020

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

Laminate structures near the north pole on Mars - Layers Exposed at North Polar Cap on Mars: Laminated structures near the north polar cap of Mars. These different layers of ice and girders correspond to climatic variations over the last ten thousand years. Image obtained on 18 April 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. At the edge of Mars' permanent North Polar cap, we see an exposure of the internal layers, each with a different mix of water ice, dust and dirt. These layers are believed to correspond to different climate conditions over the past tens of thousands of years. When we zoom in closer, we see that the distinct layers erode differently. Some are stronger and more resistant to erosion, others only weakly cemented. The strong layers form ledges

PIX4580071

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Comparison between Earth and Mars - Earth and Mars compared - Comparison at the scale of Earth and Mars sizes. The diameter of the planet Mars is half the diameter of the Earth. Mars' diameter is half that of the Earth's It has ten percent the mass If you weigh 180 pounds on Earth, you would weigh only 68 pounds on Mars. Mars is half again further from the Sun than the Earth The vast deserts of North Africa are no match for the planet-wide desert that is Mars. While the Earth is host to oceans of liquid water and has a relatively dense water-rich atmosphere, Mars is exceedingly dry, cold, and so far as we know, sterile. It is believed that Mars lost most of its water to space a long time ago, and any water that remains is frozen at the poles and locked deep in the ground as permafrost. It is an interesting coincidence that the total surface area of Mars is about the same as the surface area of dry land on the Earth

Walter B Myers

PIX4629809

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

Comparison of Earth Sizes, Venus, Mercure and Mars - Planetary-size comparison: Earth, Venus, Mercury and Mars - Earth diameter: 12 756,28 km Venus diameter: 12 100 km Mercury diameter: 4870 km March diameter: 6790 km Size comparison in diametric values: Earth: 12,756.28 km Venus: 12,100 km Mercury: 4,870 km March: 6,790 k

PIX4629876

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

Mars and Phobos seen by the Hubble space telescope -2016 - Mars with Phobos seen by the Hubble space telescope in 2016/The Tiny Moon Phobos Is Photographed During Its Quick Trip Around Mars: Image obtained on May 12, 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. Multiple poses showing the passage of the Phobos satellite around Mars. This image shows planet Mars with tiny moon Phobos on its trek around the Red Planet, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope

PIX4615036

Mars Science Laboratory- The mission in stages - Mars Science Laboratory mission stages: Mars Science Laboratory Mission Scenario (MSL). On August 6, 2012 this probe placed on the surface of the planet Mars a rover named Curiosity. This is an artist's concept of Nasa's Mars Science Laboratory Mission scenario. On August 6, 2012, the rover Curiosity has successfully landed on Gale crater

Mars Science Laboratory- The mission in stages - Mars Science Laboratory mission stages: Mars Science Laboratory Mission Scenario (MSL). On August 6, 2012 this probe placed on the surface of the planet Mars a rover named Curiosity. This is an artist's concept of Nasa's Mars Science Laboratory Mission scenario. On August 6, 2012, the rover Curiosity has successfully landed on Gale crater

Miller, Ron (b.1947)

PIX4643667

Probe Penetrator Mars 96 - Penetrator of the Mars 96 spacecraft - Cross-section view of one of the two penetrators of the Mars 96 probe. Numerous measuring instruments were incorporated. The lower part was to sink several metres into the Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Cutaway of a penetrator deployed on the martian surface showing the different experiments in the forebody and in the afterbody. The forebody should be separated from the afterbody and dive several meters into the martian soil. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

Probe Penetrator Mars 96 - Penetrator of the Mars 96 spacecraft - Cross-section view of one of the two penetrators of the Mars 96 probe. Numerous measuring instruments were incorporated. The lower part was to sink several metres into the Martian soil. Launched in 1996, the probe could not leave Earth orbit and disintegrate. Cutaway of a penetrator deployed on the martian surface showing the different experiments in the forebody and in the afterbody. The forebody should be separated from the afterbody and dive several meters into the martian soil. Launched in 1996, a rocket failure happened and the probe was desintegrated in the Earth atmosphere

D. Ducros

PIX4606433

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Sunrise on Mars. Illustration - Sunrise over a martian canyon. Artwork - Sunrise on Mars seen from a deep canyon. A blue halo surrounds the Sun, due to the presence of dust in the Martian atmosphere. This is how a martian sunrise might look from the bottom of a deep canyon. The Sun is surrounded by a bluish halo due to dust in the martian atmosphere. During the martian day, this dust absorbs the blue light from the Sun, resulting in an overall salmon colored sky, but it also scatters some of the blue light into the area immediately around the Sun. The blue color only becomes apparent near sunrise and sunset, when the light has to pass through the most amount of dust. The canyon is representative of the land forms found in the Olympica Fossae region, located in northern Tharsis, south of the Alba Patera volcano

Walter B Myers

PIX4616961

Terraformation de Mars-Vue d'artiste - Mars terraforming - Illustration - Using gigantic panels reflecting the Sun, one could melt water ice on Mars and make the planet habitable... Huge mirrors used to ice polar caps melting

Terraformation de Mars-Vue d'artiste - Mars terraforming - Illustration - Using gigantic panels reflecting the Sun, one could melt water ice on Mars and make the planet habitable... Huge mirrors used to ice polar caps melting

S. Numazawa

PIX4639642

Exploration of Mars-Illustration - Martian “” Motor Home”” - The exploration of Mars by men will require vehicles that can take a crew long distances and provide them with all the necessary protection against this hostile environment. A thorough human exploration of Mars would require some means for transporting explorers long distances over the martian surface while providing sustenance and protection from Mars' extremely inhospitable environment. This image suggests how such a martian “” motor home”” might be realized. Providing transportation and housing for a crew of two to four human explorers, this pressurized rover would provide stability, visibility, storage, and a means for generating power for locomotion and electrical systems. In this example, a pair of wing-like solar arrays atop the rover help to meet some of the energy needs, and the transparent windshield ports have been coated to shield the interior from ultraviolet light and provide additional visual contrast to the ru

Exploration of Mars-Illustration - Martian “” Motor Home”” - The exploration of Mars by men will require vehicles that can take a crew long distances and provide them with all the necessary protection against this hostile environment. A thorough human exploration of Mars would require some means for transporting explorers long distances over the martian surface while providing sustenance and protection from Mars' extremely inhospitable environment. This image suggests how such a martian “” motor home”” might be realized. Providing transportation and housing for a crew of two to four human explorers, this pressurized rover would provide stability, visibility, storage, and a means for generating power for locomotion and electrical systems. In this example, a pair of wing-like solar arrays atop the rover help to meet some of the energy needs, and the transparent windshield ports have been coated to shield the interior from ultraviolet light and provide additional visual contrast to the ru

Walter B Myers

PIX4639807

Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander

Mars: panorama of Chryse Planitia by Viking 1 - Mars: Chryse Planitia panorama by Viking 1 - Panorama of the surface of Mars obtained by the probe Viking 1 on 23 July 1976. The big rock on the left, nicknamed Big Joe, is about three metres long. Panoramic image of Chryse Planitia taken by camera 1 on the Viking 1 Lander. The image was taken on 23 July 1976, three days after Viking 1 landed. The dark rock at the left of the frame, nicknamed “” Big Joe”””, is about 3 meters across and 8 meters from the lander

Steven Hobbs

PIX4615194

Mars Exploration - Mars Exploration - Illustration: Astronauts drill the surface of Mars to find water. Astronauts drill for water on the Red Planet.

Mars Exploration - Mars Exploration - Illustration: Astronauts drill the surface of Mars to find water. Astronauts drill for water on the Red Planet.

PIX4639956

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

Comparison of Earth Sizes, Venus, Mercury and Mars - Diametre de la terre: 12,756,28 km Diametre de Venus: 12,100 km Diametre de Mercury: 4870 km Diametre de Mars: 6790 k

PIX4629886

The Colonization of Mars - Illustration - Mars Colony: Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

The Colonization of Mars - Illustration - Mars Colony: Artist's view of an inhabited base on Mars. A manned habitat on the surface of Mars

PIX4640022

Mars Jupiter Conjunction - Close conjunction between Jupiter and Mars: Astronomical bezel with in the background the bright Jupiter planets and Mars (just below) in tight conjunction. January 7, 2018. An astronomical telescope is seen in the foreground with the close conjunction between Jupiter and Mars in the background

Mars Jupiter Conjunction - Close conjunction between Jupiter and Mars: Astronomical bezel with in the background the bright Jupiter planets and Mars (just below) in tight conjunction. January 7, 2018. An astronomical telescope is seen in the foreground with the close conjunction between Jupiter and Mars in the background

Alex Conu

PIX4588288

Mars Jupiter Conjunction - Close conjunction between Jupiter and Mars: Astronomical bezel with in the background the bright Jupiter planets and Mars (just below) in tight conjunction. January 7, 2018. An astronomical telescope is seen in the foreground with the close conjunction between Jupiter and Mars in the background

Mars Jupiter Conjunction - Close conjunction between Jupiter and Mars: Astronomical bezel with in the background the bright Jupiter planets and Mars (just below) in tight conjunction. January 7, 2018. An astronomical telescope is seen in the foreground with the close conjunction between Jupiter and Mars in the background

Alex Conu

PIX4588290

Ice Towers on Mars - Illustration - Martian ice towers - Illustration: The Hellas basin on Mars would house ice towers several tens of metres high in which a geothermale activity was discovered - Unusual warm spots on Mars might represent “” ice towers””” similar to those seen in Antarctica, say researchers. ♪ They could even harbour life ♪

Ice Towers on Mars - Illustration - Martian ice towers - Illustration: The Hellas basin on Mars would house ice towers several tens of metres high in which a geothermale activity was discovered - Unusual warm spots on Mars might represent “” ice towers””” similar to those seen in Antarctica, say researchers. ♪ They could even harbour life ♪

Miller, Ron (b.1947)

PIX4617116

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

Mars - Atmosphere - View of Mars Planet with Argyre Basin, obtained by the Viking 1 probe in July 1976. Argyre measures 1300 km in diameter and is the second largest impact crater on Mars, after Hellas Planitia. The Argyre impact basin in the southern highlands of Mars. The basin, which is approximately 1,300 kilometers in diameter, was formed about 4 billion years ago during the Heavy Bombardment Period of the early Solar System when an asteroid or comet roughly 50 kilometers across impacted Mars. Argyre is believed to be the second - largest impact basin on Mars after Hellas Planitia and may be one of the best preserved ancient impact basins from the Heavy Bombardment Period

PIX4615099

Astronaut on Mars-Artist's view - Astronaut on Mars - Illustratio

Astronaut on Mars-Artist's view - Astronaut on Mars - Illustratio

S. Numazawa

PIX4639697

The Viking probe poses on Mars - Illustration - Viking landing - Artist view - Narrowly missing a fatal collision with a large rock, Viking 1 keys down on Chryse Planitia on Mars to provide the first ever closeup

The Viking probe poses on Mars - Illustration - Viking landing - Artist view - Narrowly missing a fatal collision with a large rock, Viking 1 keys down on Chryse Planitia on Mars to provide the first ever closeup

Steven Hobbs

PIX4606391

La comete Siding Spring pres de Mars - octobre 2014 - Comet Siding Spring with Mars - october 2014 - La comete C/2013 A1 Siding Spring pres la planete Mars, le 19 octobre 2014. Comet Siding Spring C/2013 A1 alongside March seen on October 19 2014

La comete Siding Spring pres de Mars - octobre 2014 - Comet Siding Spring with Mars - october 2014 - La comete C/2013 A1 Siding Spring pres la planete Mars, le 19 octobre 2014. Comet Siding Spring C/2013 A1 alongside March seen on October 19 2014

Sebastian Voltmer

PIX4571287

Mars polar cap seen by the Mariner 7 probe - The Martian polar cap as seen by the Mariner 7 spacecraft - Part of the polar cap south of Mars seen by the Mariner 7 probe in August 1969. Recolorized image. The southern martian polar cap as seen by the Mariner 7 spacecraft in august 1969. Recolorized picture

Mars polar cap seen by the Mariner 7 probe - The Martian polar cap as seen by the Mariner 7 spacecraft - Part of the polar cap south of Mars seen by the Mariner 7 probe in August 1969. Recolorized image. The southern martian polar cap as seen by the Mariner 7 spacecraft in august 1969. Recolorized picture

Steven Hobbs

PIX4615022

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

Martian dunes in Spring - March: Frost - covered dunes in crater - Detail on dunes in a crater located near the north pole of Mars. Clearly, areas covered with carbon dioxide gel appear on this image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on January 1, 2010. HIRISE is a 50 cm telescope that observes visible and near infrared Dunes are often found on crater floors. In the winter time at high northern latitudes the terrain is covered by carbon dioxide ice (dry ice). In the spring as this seasonal ice evaporates many unusual features unique to Mars are visible. On the floor of this crater where there are no dunes, the ice forms an uninterrupted layer. On the dunes however, dark streaks form as surface material from below the ice is mobilized and deposited on top of the ice. In some cases this mobile material probably slides down the steep face of the dune, while in other cases it may be literally blown out in a process of gas release similar to removing a c

PIX4616489

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

Mars - Gale Crater Region - Gale Crater area on planet Mars - View of the region of the impact crater Gale in which the Curiosity rover will be installed in 2012. This crater (in the top center of the picture) is 154 km in diameter. Image recomposed from data obtained by the Mars Global Surveyor probe. This computer - generated view depicts part of Mars at the boundary between darkness and daylight, with an area including Gale Crater beginning to catch morning light. Northward is to the left. Gale is the crater with a mound inside it near the center of the image. NASA has selected Gale as the landing site for the Mars Science Laboratory mission. The mission's rover will be placed on the ground in a northern portion of Gale crater in August 2012. Gale crater is 96 miles (154 kilometers) in diameter and holds a layered mountain rising about 3 miles (5 kilometers) above the crater floor. The intended landing site is at 4.5 degrees south latitude, 137.4 degrees east longitude. This view wa

PIX4615396

Mars and Phobos - Illustration - Mars and Phobos - Illustration: The Tharsis plateau with the Olympus Mons volcano seen from Mars's closest satellite, Phobos. Mars fills the sky of its nearest moon, tiny Phobos. Visible here are the giant volcanoes of the Tharsis region

Mars and Phobos - Illustration - Mars and Phobos - Illustration: The Tharsis plateau with the Olympus Mons volcano seen from Mars's closest satellite, Phobos. Mars fills the sky of its nearest moon, tiny Phobos. Visible here are the giant volcanoes of the Tharsis region

Miller, Ron (b.1947)

PIX4616847

Martian base-illustration - Martian base - Illustratio

Martian base-illustration - Martian base - Illustratio

L. Bret

PIX4639673

Mars with water - Artist's view - Wet Mars - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars. 3.5 billion years ago Mars had water.

Mars with water - Artist's view - Wet Mars - Artwork: More than three billion years ago, water flowed on Mars. The water is now evaporated. This illustration can also illustrate the terraformation of Mars. 3.5 billion years ago Mars had water.

PIX4616947

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

The coldest place on Mars - Coolest place on Mars: Detail of the ice cap of the southern pole of Mars, composed mainly of carbon dioxide. This dry ice accumulates on the surface mainly in winter, the temperature of this area can sometimes drop to 130 degrees Celsius below zero. Image obtained on August 29, 2016 by the HIRISE camera on board the Mars Reconnaissance orbiter probe. HIRISE is a 50 cm telescope that observes visible and near infrared. The polar cap is made from carbon dioxide (dry ice), which does not occur naturally on the Earth. The circular pits are holes in this dry ice layer that expand by a few meters each Martian year. New dry ice is constantly being added to this landscape by freezing directly out of the carbon dioxide atmosphere or falling as snow. Freezing out the atmosphere like this limits how cold the surface can get to the frost point at -130 degrees Celsius (-200 F). Nowhere on Mars can ever get any colder this, making this coolest landscape on Earth and Mars

PIX4580080

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Mars Reconnaissance Orbiter - Artist View - Mars Reconnaissance Orbiter - Artist view - The American Mars Reconnaissance Orbiter probe (MRO) was launched in August 2005 and began its observations from Mars in October 2006. Artwork of Mars Reconnaissance Orbiter (MRO) as it orbits over the martian north pole. The spacecraft was launched in August 2005 and began the first observations of March in October 2006

Steven Hobbs

PIX4606683

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Mission to Phobos - Phobos mission rocket brakes for Mars orbit - After seven months of travel, the spaceship en route to Phobos brakes to orbit around Mars. After seven months traveling from Earth to Mars the Phobos mission rocket ignites its next propellant stage in order to slow down enough to enter an orbit around Mars that will bring it to within a few miles of Phobos

Walter B Myers

PIX4639664

Martian Base - Illustration

Martian Base - Illustration

PIX5940231

European Astronaut on Mars - Illustration - European Astronaut on Mars - Illustration - A European astronaut robs the soil of March in 2030. Artist's view. An european spacewoman walking on the martian surface in 2030

European Astronaut on Mars - Illustration - European Astronaut on Mars - Illustration - A European astronaut robs the soil of March in 2030. Artist's view. An european spacewoman walking on the martian surface in 2030

P. Carril

PIX4639704

Terraformation de Mars - Illustration - Terraformed Mars - Illustration: Terraformation aims to transform the natural environment of a planet, a moon or another body, in order to bring together the conditions for a life of an earthly type, which is therefore habitable by man. The terraforming of a planet, moon or other body, is the hypothetical process of deliberately modifying its atmosphere, temperature, or ecology to be similar to those of Earth in order to make it habitable by humans. Here, astronauts on Phobos are watching martian oceans

Terraformation de Mars - Illustration - Terraformed Mars - Illustration: Terraformation aims to transform the natural environment of a planet, a moon or another body, in order to bring together the conditions for a life of an earthly type, which is therefore habitable by man. The terraforming of a planet, moon or other body, is the hypothetical process of deliberately modifying its atmosphere, temperature, or ecology to be similar to those of Earth in order to make it habitable by humans. Here, astronauts on Phobos are watching martian oceans

Miller, Ron (b.1947)

PIX4639668

Mission habitee vers Mars-Vue d'artiste - Manned mission to Mars - Artist view - Fusee a nuclear propulsion. A nuclear thermal rocket fires upon arrival in the vicinity of Mars to insert the transfer vehicle into orbit. Nuclear propulsion can shorten interplanetary trip times and can reduce the mass launched from Earth. As the primary transfer propulsion system, the spaecraft's reactor would remain inactive until departure from Earth orbit

Mission habitee vers Mars-Vue d'artiste - Manned mission to Mars - Artist view - Fusee a nuclear propulsion. A nuclear thermal rocket fires upon arrival in the vicinity of Mars to insert the transfer vehicle into orbit. Nuclear propulsion can shorten interplanetary trip times and can reduce the mass launched from Earth. As the primary transfer propulsion system, the spaecraft's reactor would remain inactive until departure from Earth orbit

PIX4639469

Snow on Mars - Illustration - Snow at the martian pole: Snow Tempete at the martian pole

Snow on Mars - Illustration - Snow at the martian pole: Snow Tempete at the martian pole

Miller, Ron (b.1947)

PIX4617063

Mars near the Full Moon-12/2007 - Full Moon with March-12/2007 - At the end of 2007, the planet Mars was closest to the Earth, it was its opposition, and it shone strong enough to remain visible to the naked eye right next to the dazzling Full Moon. Planet Mars is shining near full Moon on december 24 2007

Mars near the Full Moon-12/2007 - Full Moon with March-12/2007 - At the end of 2007, the planet Mars was closest to the Earth, it was its opposition, and it shone strong enough to remain visible to the naked eye right next to the dazzling Full Moon. Planet Mars is shining near full Moon on december 24 2007

G. Cannat

PIX4587573

Conjunction Mars Saturn and M44 - Saturn Mars conjunction - Mars, towards the center of the image, is reflected in the water; to his left Saturn near the cluster of the Creche cluster (M44). 5 June 2006, Quimper Mars (near the center left of the image) and Saturn (close to M44 star cluster) are reflecting in the water. June 5, 2006

Conjunction Mars Saturn and M44 - Saturn Mars conjunction - Mars, towards the center of the image, is reflected in the water; to his left Saturn near the cluster of the Creche cluster (M44). 5 June 2006, Quimper Mars (near the center left of the image) and Saturn (close to M44 star cluster) are reflecting in the water. June 5, 2006

Laurent Laveder

PIX4587712

Mars Exploration-Illustration - Martian Motor home - Men's exploration of Mars will require vehicles that can take a crew long distances and provide them with all the necessary protection against this hostile environment. A pressurized martian rover (AKA martian motor home) would permit human explorers to traverse long distances across the hostile martian surface from within the relative safety and comfort of a climate-controlled environment. The rover featured in this image, as seen from the rear, includes wing-like solar voltaic panels suspended above the chassis to supplement its electrical needs. Also on top is a high-gain antenna for direct communication with the Earth and various other sensors that include a long-range optical stereo telescope and meteorological instruments for monitoring the exotic climate

Mars Exploration-Illustration - Martian Motor home - Men's exploration of Mars will require vehicles that can take a crew long distances and provide them with all the necessary protection against this hostile environment. A pressurized martian rover (AKA martian motor home) would permit human explorers to traverse long distances across the hostile martian surface from within the relative safety and comfort of a climate-controlled environment. The rover featured in this image, as seen from the rear, includes wing-like solar voltaic panels suspended above the chassis to supplement its electrical needs. Also on top is a high-gain antenna for direct communication with the Earth and various other sensors that include a long-range optical stereo telescope and meteorological instruments for monitoring the exotic climate

Walter B Myers

PIX4639839

European astronauts on Mars - Illustration - European astronauts on Mars - Illustration - View of European astronauts artist near their Martian base and a mobile pressurised laboratory. European astronauts near their martian base with a mobile presurized laboratory

European astronauts on Mars - Illustration - European astronauts on Mars - Illustration - View of European astronauts artist near their Martian base and a mobile pressurised laboratory. European astronauts near their martian base with a mobile presurized laboratory

D. Ducros

PIX4639851

La conquete de Mars-Illustration - Mars outpost near mesa - Artist's view of an inhabited base on Mars. A manned habitat rests on the rocky and desolate surface of Mars. In the background is a mesa and on the right a manned rover

La conquete de Mars-Illustration - Mars outpost near mesa - Artist's view of an inhabited base on Mars. A manned habitat rests on the rocky and desolate surface of Mars. In the background is a mesa and on the right a manned rover

Walter B Myers

PIX4639947

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

Mars seen by the Hubble Space Telescope - 2016 - Mars in opposition 2016 - Image obtained on 12 May 2016 a few days before the opposition of Mars when the planet was only 80 million km away from Earth. This image shows planet Mars, as it was observed shortly before opposition in 2016, taken when the planet was 50 million miles from Earth on May 12, 2016. by the NASA/ESA Hubble Space Telescope. The photo reveals details as small as 20 miles to 30 miles across. This observation was made just a few days before March opposition on May 22, when the sun and Mars will be on exact opposite sides of Earth. Mars also will be 47.4 million miles from Earth. On May 30, Mars will be the closest it has been to Earth in 11 years, at a distance of 46.8 million miles. Some prominent features of the planet are clearly visible: the ancient and inactive shield volcano Syrtis Major; the bright and oval Hellas Planitia basin; the heavily eroded Arabia Terra in the centre of the image; the dark features of Si

PIX4614997

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

Martian dunes in Spring - March: Spring view of Dunes - Detail on sand dunes near the north pole of Mars. These dunes are covered with carbon dioxide gel during the Martian winter. In spring, dark streaks appear, sand flows caused by the degel. Image obtained by the HIRISE camera of the Mars Reconnaissance probe orbiter on April 7, 2008. HIRISE is a 50 cm telescope that observes visible and near infrared. Falling Material Kicks Up Cloud of Dust on Dunes. There is a vast region of sand dunes at high northern latitudes on Mars. In the winter, a layer of carbon dioxide ice covers the dunes, and in the spring as the sun warms the ice it evaporates. This is a very active process, and sand dislodged from the crests of the dunes cascades down, forming dark streaks. In thid image falling material has kicked up a small cloud of dust. The color of the ice surrounding adjacent streaks of material suggests that dust has settled on the ice at the bottom after similar events. Also discernible in thi

PIX4616482

Fog in a Martian Vallee - Illustration - Foggy Mars valley

Fog in a Martian Vallee - Illustration - Foggy Mars valley

Miller, Ron (b.1947)

PIX4617030

March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

March - Opportunity - Cratere Endurance. 05/2004 - Martian crater Endurance seen by Opportunity. 05/2004 - Panorama of 360 degres obtained by Opportunity from 22 to 28 May 2004. The Rover Opportunity landed on Mars in the Meridiani Planum region on January 25, 2004. This 360 - degree panorama shows “” Endurance Crater”” and the surrounding plains of Meridiani Planum on Mars. It took seven sols to complete this panorama (sols 117 - 123), using 81 separate camera positions. The composite shown here is an approximate true - color rendering

PIX4615799

Mars - Volcanoes Ceraunius Tholus and Uranius Tholus - Mosaic of images obtained by the Mars Express probe between November 25, 2004 and June 22, 2006 during three different orbits. This image shows the volcanoes Ceraunius Tholus (left) and Uranius Tholus (right). These volcanoes measure 130 and 62 km respectively, and s'elevent is 5500m and 4500m. In the second orbit, a cloud was present near the summit of Ceraunius Tholus volcano; in the final mosaic it appears cut in a straight line because the cloud had disappeared in the last image. Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. The flanks of this volcano are etched with many valleys. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. This image is derived from data acquired during three separate orbits of Mars Express, which took place between 25 November 2004 and

Mars - Volcanoes Ceraunius Tholus and Uranius Tholus - Mosaic of images obtained by the Mars Express probe between November 25, 2004 and June 22, 2006 during three different orbits. This image shows the volcanoes Ceraunius Tholus (left) and Uranius Tholus (right). These volcanoes measure 130 and 62 km respectively, and s'elevent is 5500m and 4500m. In the second orbit, a cloud was present near the summit of Ceraunius Tholus volcano; in the final mosaic it appears cut in a straight line because the cloud had disappeared in the last image. Ceraunius Tholus and Uranius Tholus are two volcanoes in the Tharsis region of Mars. Ceraunius Tholus is 130 km across and rises 5.5 km above its surroundings. The flanks of this volcano are etched with many valleys. Its neighbour, Uranius Tholus is a smaller volcano, with a base diameter of 62 km and a height of 4.5 km. This image is derived from data acquired during three separate orbits of Mars Express, which took place between 25 November 2004 and

PIX4616192

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